PPT-Status of the ESSnuSB neutrino beam and detector project

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1 Particle Physics with Neutrino Telescopes Uppsala 7 October 2019 T or d E k e löf Upp s a l a Un i v e rs i t y 20191007 PPNT in Uppsala Tord Ekelof Uppsala

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Status of the ESSnuSB neutrino beam and detector project: Transcript


1 Particle Physics with Neutrino Telescopes Uppsala 7 October 2019 T or d E k e löf Upp s a l a Un i v e rs i t y 20191007 PPNT in Uppsala Tord Ekelof Uppsala University . Naba. K . Mondal. Tata Institute of Fundamental Research. Mumbai 400005, India. Brief History. Atmospheric neutrino experiments study neutrinos produced by cosmic ray interactions in the atmosphere.. Satoshi Nakamura. Osaka University, Japan. Collaborators : H. . Kamano. (RCNP, Osaka Univ.), T. Sato (Osaka Univ.). T.-S.H. Lee (Argonne Nat’l Lab). Contents. Introduction . J. Brunner. 17/04/2013. APC. Outline. Oscillation Probabilities. Neutrino Cross Sections. The Proton Accelerator . The Neutrino Beam. Detector Performance. Event Rates / Result. Oscillation Probabilities. COSMOLOGY. EVIDENCE FOR NEW PHYSICS?. STEEN . HANNESTAD, Aarhus . University. NuHorizons. 2011. n. e. n. m. n. t. Fermion Mass Spectrum. 10. 100. 1. 10. 100. 1. 10. 100. 1. 10. 100. 1. R. e. l. d. The. d. i. A. Yu. Smirnov. Max-Planck Institute. for Nuclear Physics,. Heidelberg, Germany . NOW 2014 . September 8– 13, 2014 . . The riddle of neutrino mass:. strongly suppresses . . . Neutrinos Are Very Elusive!. We now understand that neutrinos are produced in nuclear reactions, but they were actually . predicted several decades before they were finally discovered. . O. n what basis was that prediction made?. C. Weiss. 28.11.2013. EAR2 Beam Line - Report on the Status. 1. 28.11.2013. EAR2 Beam Line - Report on the Status. 2. Beam Dump. EAR-2 Exp. Hall. 2. nd. Collimator. Magnet. Pit Shielding. Target. New Area. PPAP Meeting. Birmingham. 15 July 2009. Elisabeth Falk. University of Sussex. Def. current: running or under construction. Outline. Neutrino-oscillation experiments:. what to measure, and how. Accelerator-based experiments. Jun Cao. . Institute of High Energy Physics. ICHEP, Melbourne, July 11, . 2012. Neutrino Mixing. . 23. ~ 45. Atmospheric Accelerator. . 1. 2. ~ 34. Solar. Reactor. 0. . 1. 3. . 26. -27 May . 2014 CERN. E. . . Wildner. J. . Jonnerby. , M. . . Martini, . H. . Schönauer. . 13/03/14. EUROnuSB Lund, E. Wildner. 2. W. . . Bartmann. , E. . . Bouquerel. , . M.Dracos. , . T. . 1. Particle. Physics . with. Neutrino . Telescopes. Uppsala 7 . October. 2019. T. or. d. . E. k. e. löf. Upp. s. a. l. a. . Un. i. v. e. rs. i. t. y. 2019-10-07. PPNT in Uppsala Tord Ekelof, Uppsala University . IceCube. Justin Vandenbroucke, June 9, 2021. IceCube. Bootcamp, WIPAC, UW–Madison. Outline. Neutrino interactions and cross sections. Muon lifetime. Charged particles losing energy in matter. Ionization. Mike Sullivan. EICUG 2019. July 22-26. Paris, France . 1. Outline. Introduction. Detector Issues. Machine Issues. Unique features of the EIC. Some general questions for the detector and accelerator teams. hopes and failures. From: History of Neutrinos, Paris September 2018. For: La Physique des Neutrinos, Paris September 2022. Why am I giving this talk?. Probably because I’ve been putting out a free monthly ~100 line “long-baseline newsletter” about all things neutrino since 1992.

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